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M. Katz

Publications and source records attributed to M. Katz.

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Thresholdless Nanoscale Coaxial Lasers

The generation of coherent radiation in nanostructures has attracted considerable interest in recent years owing both to the quantum electrodynamical effects that emerge in small volumes, and to their potential for future applications. The progress towards exploring this size regime, however, has been hindered by the lack of a systematic approach to scaling down the mode as the structures shrink in size and by the high threshold power required for lasing in small cavities. Here we present a new family of metamaterial-like nano-cavities consisting of metallic coaxial nanostructures that solves both of these problems. The proposed nanoscale coaxial cavities can operate as thresholdless lasers, and their size is not restricted by the mode cut-off. Using these new nano-cavities we have succeeded to demonstrate for the first time thresholdless lasing in a broadband gain medium, and the smallest room temperature, continuous wave, telecom laser to date. The nanoscale coaxial cavities are the first systematic step towards unveiling the potentials of ultra small quantum electrodynamical objects in which atom-field interactions generate new functionalities.

physics.optics

Supernova Remnants and Star Formation in the Large Magellanic Cloud

It has often been suggested that supernova remnants (SNRs) can trigger star formation. To investigate the relationship between SNRs and star formation, we have examined the known sample of 45 SNRs in the Large Magellanic Cloud to search for associated young stellar objects (YSOs) and molecular clouds. We find seven SNRs associated with both YSOs and molecular clouds, three SNRs associated with YSOs but not molecular clouds, and eight SNRs near molecular clouds but not associated with YSOs. Among the 10 SNRs associated with YSOs, the association between the YSOs and SNRs can be either rejected or cannot be convincingly established for eight cases. Only two SNRs have YSOs closely aligned along their rims; however, the time elapsed since the SNR began to interact with the YSOs' natal clouds is much shorter than the contraction timescales of the YSOs, and thus we do not see any evidence of SNR-triggered star formation in the LMC. The 15 SNRs that are near molecular clouds may trigger star formation in the future when the SNR shocks have slowed down to <45 km/s. We discuss how SNRs can alter the physical properties and abundances of YSOs.

astro-ph.GA